[meteorite-list] Ghubara Revisited
From: Dan Fronefield <dfronfld_at_meteoritecentral.com>
Date: Thu Apr 22 09:37:34 2004 Message-ID: <3.0.6.32.20001214200648.00b86b80_at_hiwaay.net> Well, I couldn't find my loupe and my scanner is still dead so I can't send pics. But visually (unaided) it still seems as if the the lighter matrix has more defined chondrules. Obviously, this could be an artifact of limited magnification.....near sightedness.....color blindness.....oh heck, I give up.......when I poke it with my white cane, it all looks alike <G>. I'll have to unpack my stereo microscope to take a "real" look at it. So.....if Ghubara is prone to rusting, what is the prefered treatment? (I have mine soaking in alcohol at the moment) Thanks Dan At 12:00 AM 12/15/00 +0100, you wrote: >Dan wrote: > >> The lighter colored section also seemed >> to have more defined chondrules. > >Bernd responded: > >> a regolith breccia with a dark matrix and light >> clasts. The lighter colored sections have more >> defined chondrules because there are L3 frag- >> ments set in an L5 host. > >James Baxter (private mail): > >> I recently obtained a slice of Ghubara in which the DARK >> portion appears to be unequilibrated and has prominent >> chondrules and the light portion looks more equilibrated >> and has fewer and less distinct chondrules. This seems to >> be the reverse of what you described. > >Hello List, > >James' observations are confirmed by a passage from Wasson's 1974 book >on meteorites [WASSON J.T. (1974) Meteorites, Springer Verlag 1974, p. >196]: > >"The difference in petrologic grade between xenoliths and host may be >related to their relative friabilities. The material of lower petrologic >type was more friable and was comminuted to form the host; the stronger >materials of higher petrologic type were fragmented, but generally >survived as larger clasts." > >Lower petrologic type obviously implies more chondrules - thus the dark >Ghubara matrix should show abundant chondrules. James' scanned picture >clearly shows just that and so does a look at my specimen. Higher >petrologic type means a higher degree of recrystallization, and, >consequently fewer chondrules. In a nutshell: The host matrix is >chondrule-rich, the clasts should be chondrule-poor. > >But Dan wrote to the List: > >> The lighter colored section also seemed >> to have more defined chondrules. > >Perhaps Wasson can again help (page 196): > >"If this explanation is correct, some cases should be found where the >clast is of lower petrologic type than the host, since the correlation >between friability and petrologic type is not a perfect one." > >Wasson does not mention if such "cases" may occur simultaneously in one >and the same meteorite (specimen). Does James have the "run-of-the-mill" >version of Ghubara and Dan the more "exotic" version? Or is Dan >mistaken? > >With the help of a 12x loupe, I took another look at my Ghubara slice >and noticed about an equal number of chondrules in both "lithologies", >whereas James' xenolithic component almost seems to be devoid of any >chondrules; so now I am at my wit's end :-( > >Folks, grab your Ghubaras, look at them closely, take your Ghubara thin >sections and examine them in plane and polarized light and report to the >list your findings. I think this is a great occasion for this list to do >invaluable scientific, observational work. > >By the way, the entry in the Blue Book also supports James' observation: > >"... the host is unequilibrated, with olivine Fa21.6 >to Fa26.5, but olivine of xenoliths is Fa24 ..." > > >Best wishes and >thank you very >much James, > >Bernd Handmade Knives by D. Fronefield "Specializing in meteorites and other exotic materials" http://hiwaay.net/~dfronfld Received on Thu 14 Dec 2000 08:06:48 PM PST |
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